Bulge dwarfs and subgiants abundances from (Bensby et al. 2013colored circles), overlaid on stars of the solar vicinity from (Bensby et al. 2014 gray and black dots) for alpha elements (Mg + Si + Ti), Al, Ba, Na, Ni. The bulge data for La and Eu comes from Van der Swaelmen et al. (2016). Stars from Bensby et al. (2014) belonging to the inner disk sequence stars (and which are expected to contribute to the bulge) are selected using alpha abundances by choosing those above the black line in the plot (a). Discarding the outer disk objects (those below the line), the overlap between the inner disk stars of the solar vicinity and bulge stars is excellent. Colors and sizes of the symbols for bulge stars is coding their ages, which come from Bensby et al. (2013).